Narrow band observations of Titan at selected wavelengths in the 8-13 micron range show evidence for a strong temperature inversion and the existence of at least one more spectroscopically active component in the atmosphere in addition to H2 and CH4.
The 8-13 micron observations of Titan
1974-01-01
Conference paper
No indication
English
NTRS | 1992
|ISO Observations of Titan with SWS/Grating
British Library Online Contents | 1997
|Observations of Titan IIIC Transtage Fragmentation Debris
British Library Conference Proceedings | 2014
|Voyager photopolarimeter observations of Saturn and Titan
Elsevier | 1983
|